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dc.contributor.authorGardiner, Nicholas J.
dc.contributor.authorKirkland, Christopher L.
dc.contributor.authorHollis, Julie A.
dc.contributor.authorCawood, Peter A.
dc.contributor.authorNebel, Oliver
dc.contributor.authorSzilas, Kristoffer
dc.contributor.authorYakymchuk, Chris
dc.date.accessioned2020-01-29T09:30:08Z
dc.date.available2020-01-29T09:30:08Z
dc.date.issued2020-03-15
dc.identifier266070594
dc.identifier6b0039d4-3f64-45a2-bdfe-9cda3e5ea970
dc.identifier85077932606
dc.identifier000515198200022
dc.identifier.citationGardiner , N J , Kirkland , C L , Hollis , J A , Cawood , P A , Nebel , O , Szilas , K & Yakymchuk , C 2020 , ' North Atlantic Craton architecture revealed by kimberlite-hosted crustal zircons ' , Earth and Planetary Science Letters , vol. 534 , 116091 . https://doi.org/10.1016/j.epsl.2020.116091en
dc.identifier.issn0012-821X
dc.identifier.otherRIS: urn:7B28006A8A7A712182FF47C1F9C2D8D1
dc.identifier.otherORCID: /0000-0003-3465-9295/work/68281984
dc.identifier.urihttps://hdl.handle.net/10023/19368
dc.descriptionThe Maniitsoq project is supported by the Ministry of Mineral Resources, Government of Greenland. NJG and PAC thank Australian Research Council grant FL160100168 for financial support. ON is supported by Australian Research Council grant FT140101062 and the Melbourne TIE team.en
dc.description.abstractArchean cratons are composites of terranes formed at different times, juxtaposed during craton assembly. Cratons are underpinned by a deep lithospheric root, and models for the development of this cratonic lithosphere include both vertical and horizontal accretion. How different Archean terranes at the surface are reflected vertically within the lithosphere, which might inform on modes of formation, is poorly constrained. Kimberlites, which originate from significant depths within the upper mantle, sample cratonic interiors. The North Atlantic Craton, West Greenland, comprises Eoarchean and Mesoarchean gneiss terranes – the latter including the Akia Terrane – assembled during the late Archean. We report U–Pb and Hf isotopic, and trace element, data measured in zircon xenocrysts from a Neoproterozoic (557 Ma) kimberlite which intruded the Mesoarchean Akia Terrane. The zircon trace element profiles suggest they crystallized from evolved magmas, and their Eo- to Neoarchean U–Pb ages match the surrounding gneiss terranes, and highlight that magmatism was episodic. Zircon Hf isotope values lie within two crustal evolution trends: a Mesoarchean trend and an Eoarchean trend. The Eoarchean trend is anchored on 3.8 Ga orthogneiss, and includes 3.6–3.5 Ga, 2.7 and 2.5–2.4 Ga aged zircons. The Mesoarchean Akia Terrane may have been built upon mafic crust, in which case all zircons whose Hf isotopes lie within the Eoarchean trend were derived from the surrounding Eoarchean gneiss terranes, emplaced under the Akia Terrane after ca. 2.97 or 2.7 Ga, perhaps during late Archean terrane assembly. Kimberlite-hosted peridotite rhenium depletion model ages suggest a late Archean stabilization for the lithospheric mantle. The zircon data support a model of lithospheric growth via tectonic stacking for the North Atlantic Craton.
dc.format.extent2422640
dc.language.isoeng
dc.relation.ispartofEarth and Planetary Science Lettersen
dc.subjectlamprophyreen
dc.subjectArchean Archaeanen
dc.subjectGreenlanden
dc.subjectItsaq Isuaen
dc.subjectIsukasia Akia Terraneen
dc.subjectSCLM lithosphere mantleen
dc.subjectGE Environmental Sciencesen
dc.subjectQE Geologyen
dc.subjectDASen
dc.subject.lccGEen
dc.subject.lccQEen
dc.titleNorth Atlantic Craton architecture revealed by kimberlite-hosted crustal zirconsen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Earth & Environmental Sciencesen
dc.identifier.doi10.1016/j.epsl.2020.116091
dc.description.statusPeer revieweden


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